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20082026
most citedThe Zwicky Transient Facility: System Overview, Performance, and First Results

2.1k citations · 11.3k across the 86 of their papers we have counts for

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Showing 2019Show all

12 papers · 1 filter

astro-ph.HE2019★ 9 cited

The Zwicky Transient Facility Bright Transient Survey I: Spectroscopic Classification and the Redshift Completeness of Local Galaxy Catalogs

U. C. Fremling, A. A. Miller, Y. Sharma +37

The Zwicky Transient Facility (ZTF) is performing a three-day cadence survey of the visible Northern sky (~3). The transient candidates found in this survey are announced via pu…

astro-ph.HE2019★ 106 cited

ZTF Early Observations of Type Ia Supernovae I: Properties of the 2018 Sample

Yuhan Yao, Adam A. Miller, S. R. Kulkarni +32

Early-time observations of Type Ia supernovae (SNe Ia) are essential to constrain their progenitor properties. In this paper, we present high-quality light curves of 127 SNe Ia dis…

astro-ph.CO2019★ 55 cited

SUGAR: An improved empirical model of Type Ia Supernovae based on spectral features

P. -F. Léget, E. Gangler, F. Mondon +40

Type Ia Supernovae (SNe Ia) are widely used to measure the expansion of the Universe. Improving distance measurements of SNe Ia is one technique to better constrain the acceleratio…

astro-ph.HE2019★ 27 cited

SN 2012dn from early to late times: 09dc-like supernovae reassessed

S. Taubenberger, A. Floers, C. Vogl +40

As a candidate 'super-Chandrasekhar' or 09dc-like Type Ia supernova (SN Ia), SN 2012dn shares many characteristics with other members of this remarkable class of objects but lacks…

astro-ph.IM2019★ 102 cited

Transient processing and analysis using : Alert Management, Photometry and Evaluation of Lightcurves

J. Nordin, V. Brinnel, J. van Santen +18

Both multi-messenger astronomy and new high-throughput wide-field surveys require flexible tools for the selection and analysis of astrophysical transients. We here introduce the A…

astro-ph.CO2019★ 17 cited

Testing Gravity Using Type Ia Supernovae Discovered by Next-Generation Wide-Field Imaging Surveys

A. G. Kim, G. Aldering, P. Antilogus +29

In the upcoming decade cadenced wide-field imaging surveys will increase the number of identified Type~Ia supernovae (SNe~Ia) from the hundreds to the hundreds of thousands…

astro-ph.IM2019★ 148 cited

A Fully Automated Integral Field Spectrograph Pipeline for the SEDMachine: pysedm

M. Rigault, J. D. Neill, N. Blagorodnova +8

Current time domain facilities are discovering hundreds of new galactic and extra-galactic transients every week. Classifying the ever-increasing number of transients is challengin…

astro-ph.IM2019★ 850 cited

The Zwicky Transient Facility: Science Objectives

Matthew J. Graham, S. R. Kulkarni, Eric C. Bellm +114

The Zwicky Transient Facility (ZTF), a public-private enterprise, is a new time domain survey employing a dedicated camera on the Palomar 48-inch Schmidt telescope with a 47 deg$^2…

astro-ph.IM2019★ 139 cited

Machine Learning for the Zwicky Transient Facility

Ashish Mahabal, Umaa Rebbapragada, Richard Walters +47

The Zwicky Transient Facility is a large optical survey in multiple filters producing hundreds of thousands of transient alerts per night. We describe here various machine learning…

astro-ph.IM2019★ 2.1k cited

The Zwicky Transient Facility: System Overview, Performance, and First Results

Eric C. Bellm, Shrinivas R. Kulkarni, Matthew J. Graham +112

The Zwicky Transient Facility (ZTF) is a new optical time-domain survey that uses the Palomar 48-inch Schmidt telescope. A custom-built wide-field camera provides a 47 deg fiel…

astro-ph.IM2019★ 43 cited

: Estimating Transient Discovery Rates for the Zwicky Transient Facility

Ulrich Feindt, Jakob Nordin, Mickael Rigault +4

When planning a survey for astronomical transients, many factors such as cadence, filter choice, sky coverage, and depth of observations need to be balanced in order to optimize th…

astro-ph.HE2019★ 19 cited

Search for transient optical counterparts to high-energy IceCube neutrinos with Pan-STARRS1

E. Kankare, M. Huber, S. J. Smartt +345

In order to identify the sources of the observed diffuse high-energy neutrino flux, it is crucial to discover their electromagnetic counterparts. IceCube began releasing alerts for…